相关实验视频
Updated: Jul 19, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
太阳系外行星upsilon Andromedae b b的相位依赖的红外亮度
Joseph Harrington1, Brad M Hansen, Statia H Luszcz
1Department of Physics, University of Central Florida, Orlando, FL 32816, USA.
概括
环绕upsilonAndromedae轨道的最内层行星呈现出炎热的白天侧面和寒冷的夜晚侧面. 斯皮策太空望远镜的观测显示,这种温度差异是由于它与宿主恒星的距离近.
科学领域:
- 外系行星科学 外系行星科学
- 红外天文学 红外天文学
- 恒星系统研究 恒星系统研究
背景情况:
- 乌普西隆·安德罗米达星有三个已知的行星系统.
- 最内在的行星的轨道周期很短 (4.617天),质量很大 (≥0.69木星质量).
- 这颗系外行星与其恒星的接近导致吸收的辐射超过了内部热量产生.
研究的目的:
- 为了研究Upsilon Andromedae系统中最内在的行星的热特性.
- 在系外行星表面呈现温度不对称的观测证据.
- 为了利用红外光曲线数据进行系外行星大气研究.
主要方法:
- 使用斯皮策太空望远镜观测Upsilon的安德罗米达星系.
- 获取和分析24微米红外光线曲线.
- 光曲线变化与最内在行星的轨道相的相关性.
主要成果:
- 在24微米光曲线中检测到明显的相变化.
- 观察到的变化直接对应于最内在的行星的轨道运动.
- 这表明行星的子星 (白天) 和反星 (夜晚) 两侧之间存在显著的温度差异.
结论:
- 靠近宿主恒星的系外行星可以表现出极端的昼夜温度对比.
- 最内在的上层行星Andromedae的子星面比它的反星面要热得多.
- 红外观测为描述系外行星热环境提供了强大的工具.
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